OAI/Analysis/KadisonKastler/SpectralRecovery.lean
7 declarations, 0 contain sorry, 0 declared as axioms
Turning scalar spectral tails into compressed recovery estimates
- def
OAI.KadisonKastler.ProjectionTraceIndependentline 17Source documentation
The degree-two consequence of freeness used for the tail estimate.
def ProjectionTraceIndependent (τ : FaithfulTracialState B) (p : B) (A : StarSubalgebra ℂ B) : Prop := …Mentions: OAI.KadisonKastler.FaithfulTracialState
- theorem
OAI.KadisonKastler.traceTwoNorm_projection_left_sqline 21 - theorem
OAI.KadisonKastler.traceTwoNorm_projection_right_sqline 36 - theorem
OAI.KadisonKastler.spectral_tail_factor_normsline 53Source documentation
The left and right factors in the tail Hölder estimate have the same squared two-norm, equal to the scalar tail divided by the matrix size.
theorem spectral_tail_factor_norms (τ : FaithfulTracialState B) {A : StarSubalgebra ℂ B} {p f e : B} {n : ℕ} (hp : IsStarProjection p) (he : IsStarProjection e) (hf : f ∈ A) (heA : e ∈ A) (hfe : Commute f e) (hpτ : τ.toLinearMap p = (((n : ℝ)⁻¹ : ℝ) : ℂ)) (hind : ProjectionTraceIndependent τ p A) : traceTwoNorm τ (p * f * (1 - e)) ^ 2 = (n : ℝ)⁻¹ * (τ.toLinearMap (star f * f * (1 - e))).re ∧ traceTwoNorm τ ((1 - e) * f * p) ^ 2 = (n : ℝ)⁻¹ * (τ.toLinearMap (star f * f * (1 - e))).re := by …Mentions: OAI.KadisonKastler.FaithfulTracialState, OAI.KadisonKastler.ProjectionTraceIndependent, OAI.KadisonKastler.traceTwoNorm
- theorem
OAI.KadisonKastler.compressed_spectral_tail_leline 98Source documentation
Freeness removes the factor
nfrom the one-norm tail of the compressed square. Only the scalar Haar tail remains.theorem compressed_spectral_tail_le (τ : FaithfulTracialState B) {A : StarSubalgebra ℂ B} {p f e : B} {n : ℕ} (hn : 0 < n) (hp : IsStarProjection p) (he : IsStarProjection e) (hf : f ∈ A) (heA : e ∈ A) (hfe : Commute f e) (hpτ : τ.toLinearMap p = (((n : ℝ)⁻¹ : ℝ) : ℂ)) (hind : ProjectionTraceIndependent τ p A) : (n : ℝ) * traceOneNorm τ (recoveryCompression p f - p * e * (f * f) * e * p) ≤ (τ.toLinearMap (star f * f * (1 - e))).re := by …Mentions: OAI.KadisonKastler.FaithfulTracialState, OAI.KadisonKastler.ProjectionTraceIndependent, OAI.KadisonKastler.traceOneNorm, OAI.KadisonKastler.recoveryCompression
- theorem
OAI.KadisonKastler.normal_compressed_square_massline 122Source documentation
For a normal polynomial the absolute value of its compressed square is precisely the compressed energy.
theorem normal_compressed_square_mass (τ : FaithfulTracialState B) {f e : B} (hf : IsStarNormal f) (he : IsStarProjection e) (hfe : Commute f e) : traceOneNorm τ (e * (f * f) * e) = (τ.toLinearMap (star f * f * e)).re := by …Mentions: OAI.KadisonKastler.FaithfulTracialState, OAI.KadisonKastler.traceOneNorm
- theorem
OAI.KadisonKastler.normal_compressed_square_mass_lowerline 138Source documentation
Unit total energy and a scalar tail bound give the mass hypothesis in scalar recovery, without another analytic estimate.
theorem normal_compressed_square_mass_lower (τ : FaithfulTracialState B) {f e : B} {tail : ℝ} (hf : IsStarNormal f) (he : IsStarProjection e) (hfe : Commute f e) (hunit : τ.toLinearMap (star f * f) = 1) (htail : (τ.toLinearMap (star f * f * (1 - e))).re ≤ tail) : 1 - tail ≤ traceOneNorm τ (e * (f * f) * e) := by …Mentions: OAI.KadisonKastler.FaithfulTracialState, OAI.KadisonKastler.traceOneNorm